(Q59061964)

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Observational lower mass limit for black hole formation derived from massive X-ray binaries

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Observational lower mass limit for black hole formation derived from massive X-ray binaries (English)

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E. P. J. van den Heuvel

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1

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G. M. H. J. Habets

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2

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English

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June 1984

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309

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5969

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598–600

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https://scigraph.springernature.com/pub.10.1038/309598a0

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Discovery of a massive unseen star in LMC X-3

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Mass of Large Magellanic Cloud X-3

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Hydrodynamic effects of a stellar explosion on a binary companion star

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7 January 2021

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On the tidal spin up and orbital circularization rate for the massive X-ray binary systems

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Approximations to the radii of Roche lobes

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Double core evolution. I. A 16 solar M star with a 1 solar M neutron star companion

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Mass loss from O and B stars

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7 January 2021

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The orbital period of 2S 1223-624 (GX 301-2)

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A determination of the orbit of GX 301-2

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The initial mass function for massive stars

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1014556629

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(Q59061964)

Observational lower mass limit for black hole formation derived from massive X-ray binaries

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